Superfluidity in beta-stable neutron star matter

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dc.creatorElgaroey, Oe.
dc.creatorEngvik, L.
dc.creatorHjorth-Jensen, M.
dc.creatorOsnes, E.
dc.date1996-04-25
dc.date.accessioned2026-07-07T12:33:17Z
dc.date.available2026-07-07T12:33:17Z
dc.descriptionIn this work we present results for pairing gaps in $β$--stable neutron star matter with electrons and muons using a relativistic Dirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange models for the nucleon--nucleon interaction. Results are given for superconducting $^1S_0$ protons and $^3P_2$ and $^1D_2$ neutron superfluids. A comparison is made with recent non--relativistic calculations and the implications for neutron star cooling are discussed.
dc.description7 pages, RevTex latex style, 3 figs included
dc.identifierhttps://arxiv.org/abs/nucl-th/9604041
dc.identifierhttp://arxiv.org/abs/nucl-th/9604041
dc.identifierPhys.Rev.Lett.77:1428-1431,1996
dc.identifierdoi:10.1103/PhysRevLett.77.1428
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/217074
dc.subjectNuclear Theory
dc.titleSuperfluidity in beta-stable neutron star matter
dc.typetext

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